The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The color profile appears to be relatively homogenous, dominated by yellow-red hues, suggesting a population of older stars and a lack of significant ongoing star formation. The galaxy exhibits a high degree of roundness. There is no discernible evidence of spiral arms or a disk-like structure. The galaxy's structure does not indicate any major merger events, nor does it appear to be significantly disturbed. There may be a small chance of a minor disturbance. The size of the galaxy is intermediate.
