The galaxy appears to be a relatively compact object, exhibiting a generally smooth morphology with some features. There's a central, bright, concentrated bulge from which a faint, diffuse disk extends. The bulge region is likely dominated by an older stellar population, suggested by its redder color. The disk exhibits a bluer hue, potentially indicating ongoing or recent star formation within its spiral arms or patchy regions. There's no obvious bar structure visible. There is no indication of a major merger in progress. The shape is mostly round.
