The galaxy appears as an elliptical or lenticular type, exhibiting a generally smooth morphology. Its central bulge region is bright and concentrated, indicating a high density of stars, likely older populations. The color gradients suggest a stellar population that is redder in the core and slightly bluer in the outer regions. There is an apparent disk of stars that extends to the side of the bulge, but is relatively faint and undisturbed. The galaxy shows no clear signs of active star formation or ongoing major mergers. There is a slight asymmetry in the shape of the outer regions of the galaxy, possibly indicating a minor interaction or tidal disturbance.