The galaxy presents as a slightly oblong, diffuse object with a brighter, concentrated central bulge. The color profile suggests a redder core, indicative of an older stellar population. The surrounding disk exhibits a bluer hue, hinting at ongoing star formation. While the galaxy appears mostly smooth, subtle variations in color and intensity suggest possible faint, poorly defined spiral structures or patchy star-forming regions within the disk. The galaxy's shape is most likely in between round and cigar shaped. There is no strong evidence of a major merger. Based on the colors and features, it is possibly an early-type spiral or a late-type lenticular galaxy undergoing moderate star formation.
