This galaxy appears to be a spiral galaxy, viewed at a high inclination. It is characterized by a bright, yellowish central bulge, possibly indicating an older stellar population concentrated in the core. Extending outwards from the bulge, there are hints of spiral arm structure, though these are not sharply defined. The arms exhibit a bluer color, suggestive of ongoing star formation. The overall morphology leans towards a more elliptical shape, possibly resembling a lenticular galaxy. There is no visually evident sign of major tidal disruption or ongoing major merger activity, however some fainter areas could indicate minor disturbances.
