The galaxy appears to be a relatively smooth, somewhat elongated structure. It exhibits a concentrated central bulge with a yellowish hue, possibly indicating an older stellar population dominating this region. Extending outward from the bulge is a fainter, more diffuse disk component that displays a bluish color. The blue suggests ongoing star formation, although it seems minimal. Overall, the galaxy's morphology leans towards an elliptical, but with hints of a disk structure. There is no obvious presence of strong tidal features or major disturbances. There is no indication of intense star formation. It is possible that the galaxy is in transition, evolving from a spiral towards a more elliptical morphology.
