The galaxy presents as a somewhat face-on spiral with a smooth, diffuse appearance. The core exhibits a bright, concentrated region. The disk component shows a moderate level of internal structure. The galaxy has an elliptical shape. The spiral arms are not well-defined. The color gradient suggests a moderate population of older stars, with some evidence of ongoing or recent star formation, particularly in the central bulge. There may be signs of a weak tidal interaction. There are some minor disturbances with the galaxy but it doesn't appear to be a full merger. 
