The galaxy appears to be a relatively smooth, elongated elliptical type. Its overall shape is cigar-like and the light is concentrated toward the center, indicating a possible bulge. The lack of distinct spiral arms or a pronounced disk further suggests an elliptical classification. 

Color gradients indicate varying stellar populations or dust content. The central region exhibits a slightly yellowish-white hue, potentially indicating older, cooler stars. The outer regions of the galaxy display hints of a bluer color, possibly arising from a younger stellar population.

There is no obvious evidence of active galactic nuclei activity or strong ongoing star formation from the color profile. No major signs of recent mergers, tidal tails, or strong distortions are apparent, although a slight asymmetry might suggest minor interaction.
