The galaxy appears to be a lenticular or elliptical type, exhibiting a generally smooth, featureless morphology. It presents an elongated shape, possibly leaning towards a cigar-like appearance. The light distribution suggests a central bulge, with a gradual decrease in luminosity towards the outer edges. The color profile is dominated by a yellowish-orange hue, implying an older stellar population with fewer young, blue stars. There are no apparent signs of active star formation regions or spiral arm structures within the visible spectrum. No significant tidal disturbances or close companion galaxies are observed, suggesting a relative state of isolation and dynamical stability.
