The galaxy presents a generally smooth, elongated morphology, exhibiting a cigar-like shape. Its core region is a bright, concentrated area of light with an off-white or yellow hue, suggesting a significant population of older stars. Fainter, bluer light is also present in the galaxy, indicating a lesser population of young, hot stars and ongoing star formation. The galaxy does not appear to have a pronounced disk or spiral arms. There is no visible evidence of tidal tails or distorted morphology indicative of major merging events. Instead, the morphology is likely the result of a minor merger or interaction. Overall, the galaxy seems to be a sizable, massive system.