The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The luminosity appears to gradually decrease from the core outwards, with no distinct spiral arm features visible. The galaxy exhibits a predominantly yellow-red color profile, indicating a population of older stars and a lower rate of ongoing star formation. There is no discernible evidence of significant tidal disturbances or mergers with other galaxies. The general morphology suggests that this is an elliptical galaxy, likely with a substantial stellar mass.
