The galaxy appears as a relatively smooth, oval-shaped structure. It exhibits a bright central region, possibly indicative of an active galactic nucleus or a dense stellar population. There are subtle color gradients, with a slightly bluer hue towards the outer edges, which could suggest ongoing star formation in those regions. However, the overall smoothness and lack of prominent spiral arms or significant dust lanes suggest it may be an early-type spiral galaxy, or possibly an elliptical galaxy with some residual star formation. There is no apparent major ongoing merger activity or signs of strong tidal disruption. However, there is a slight distortion in its shape which may be indicative of a minor merger event in the past or present.
