The galaxy presents an elongated, cigar-shaped morphology, with a noticeable central bulge. The light distribution is relatively smooth, yet subtle features hint at a possible disk component. The color gradient indicates a concentration of older stars within the central bulge, exhibiting a yellowish hue. Fainter, bluer regions at the edges of the galaxy suggests more recent or ongoing star formation. There is evidence of a possible minor disturbance or interaction, as one end of the galaxy appears slightly irregular or elongated. Overall, this galaxy appears to be an intermediate mass galaxy undergoing moderate star formation, with a notable bulge and hints of a disk structure. The possibility of it being involved in a past or ongoing minor merger event can't be discounted.
