The galaxy exhibits a generally elliptical morphology, displaying a smooth, centrally concentrated bulge. The light distribution suggests a relatively high Sersic index, indicative of an older stellar population and a more evolved system. The galaxy appears slightly elongated, with the semi-major axis oriented at roughly 50 degrees. The color profile reveals a redder central region, likely due to the presence of older, cooler stars and dust. Fainter, bluer regions are discernible in the outer parts of the galaxy, suggesting some level of ongoing or recent star formation, although it does not appear vigorous. There appears to be some minor disturbance, possibly hinting at a past or ongoing interaction.
