This galaxy appears to be a relatively small, well-defined disc galaxy, likely seen at a high inclination angle close to face-on. The central bulge is bright and concentrated, exhibiting a noticeably bluer hue compared to the outer regions of the disc, indicative of a younger stellar population or ongoing star formation. The surrounding disc shows spiral structure with hints of asymmetry. The galaxy's light profile seems relatively smooth. There is evidence of tidal disturbance in the disk, potentially indicating a past or ongoing merger event.
