The galaxy presents as an elongated, somewhat cigar-shaped structure. It appears to have a dominant central bulge, which exhibits a yellowish-white hue, possibly indicative of an older stellar population. Surrounding the bulge is a disk component, displaying a bluer color. This suggests the presence of younger, hotter stars and ongoing star formation, although not at a substantial rate. The outer edges of the disk appear smooth and less structured, with no prominent spiral arm features visible in this image. Overall, the galaxy appears relatively undisturbed, showing no significant signs of recent major mergers or tidal interactions. The light distribution is moderately concentrated, with a gradual decline in brightness from the bulge outwards.
