This galaxy exhibits a generally smooth morphology, suggesting an elliptical or lenticular type. There's a moderately concentrated central bulge, giving way to a fainter, more diffuse halo extending outwards. Some features disrupt the overall smoothness of the galaxy. A faint tidal tail extends from the main body, possibly indicative of past or ongoing gravitational interactions. Within the central region, there appears to be some distinct, irregular structure, perhaps a dust lane or a region of active star formation. The core of the galaxy has a relatively uniform color profile, which may indicate an older stellar population. Overall, the galaxy exhibits characteristics suggestive of a post-merger system that is gradually settling into a more stable configuration.
