The galaxy presents an overall elliptical morphology, although there's evidence of a disk-like structure. The color distribution indicates a predominantly older stellar population, particularly concentrated in the central bulge region. There's a subtle color gradient, shifting towards bluer hues away from the center, suggesting the presence of younger stars in the outer regions. The galaxy exhibits an axial ratio of approximately 0.6, indicating that it is somewhat flattened. There are no prominent spiral arm features visible, instead it appears largely smooth. Its isophotes exhibit slight twisting, potentially hinting at past interactions. The presence of neutral hydrogen is confirmed, and the spectral width measurements indicate rotational motion. The estimated hydrogen mass suggests a normal gas content for a galaxy of its type. Star formation activity appears to be relatively low overall, though slightly higher in the disk relative to the central bulge. No major signs of significant recent merger activity are observed, though some evidence of minor disturbances exists.
