The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and concentrated morphology. The central bulge region is prominent and displays a yellowish-white hue, suggesting an older stellar population dominating this area. Surrounding the bulge, there is a more diffuse, somewhat flattened disk-like component visible. This outer region shows a bluer color, hinting at the presence of younger, hotter stars and possibly ongoing star formation, though at a relatively low rate. There is subtle asymmetry in the distribution of the bluer component, potentially indicative of a past or minor merger event causing slight disturbances in the galaxy's overall structure. The galaxy does not present any prominent spiral arm features or significant tidal tails. It appears relatively isolated in its environment.
