The galaxy presents as an elliptical morphology, although a slight disk-like structure cannot be completely ruled out. The central bulge is prominent, exhibiting a smooth, concentrated distribution of light. The outer regions display a more diffuse character, gradually fading into the background sky. The major axis of the galaxy appears to be oriented at an angle with respect to the line of sight, indicating a tilted or inclined view. There is no evidence of strong spiral arm structure or significant dust lanes within the visible spectrum. The overall color profile suggests a relatively mature stellar population, consistent with an older galaxy. Slight asymmetry may suggest some tidal interaction.
