The galaxy presents an elliptical morphology, elongated with a high degree of axial ratio. The central bulge is prominent, displaying a concentrated luminosity profile. A slight deviation from perfect smoothness is observed in the outer regions. The galaxy's color index suggests a relatively evolved stellar population, with a tendency towards redder hues indicative of older stars and reduced star formation. There is no clear indication of spiral arms or active star-forming regions, reinforcing the classification of an elliptical type. The galaxy exhibits a smooth light distribution from the nucleus outward, gradually decreasing in intensity towards the edge.
