The galaxy presents a largely smooth, elliptical morphology. It is characterized by a concentrated central bulge that appears nearly spherical. The light profile is notably diffuse towards the outer edges, exhibiting a smooth transition without distinct spiral arm features or prominent dust lanes. The color gradient suggests a dominant population of older stars, with a yellowish hue indicative of relatively low ongoing star formation. There are no visually apparent signs of tidal disturbances or recent merger activity. Overall, the galaxy appears to be a relatively quiescent, evolved system.
