The galaxy presents as a relatively smooth, disk-shaped structure. It exhibits a moderate central bulge with a gradually decreasing luminosity outwards. The overall color appears yellowish, suggesting an older stellar population. There is some indication of spiral arm structure, though it is not sharply defined. No strong signs of active star formation are immediately apparent, but there are hints of slightly bluer regions within the disk. There is no evidence of any major mergers or strong tidal disturbances. The galaxy appears to be a relatively undisturbed system, likely a late-type spiral transitioning to an earlier type.