The galaxy presents a distinct, elongated morphology, closely resembling a cigar shape. Its light profile indicates a relatively smooth distribution, suggesting a lack of prominent spiral arm structures or significant dust lanes visible at this resolution. The central region appears brighter and exhibits a yellowish hue, potentially indicative of an older stellar population. Moving outward, the galaxy's color transitions to a bluer tint, particularly towards the edges, which could be due to the presence of younger, hotter stars. The overall structure suggests a system dominated by bulge-like components, with only subtle hints of any disk structure. There is very faint evidence of minor disturbances to the galaxy's structure. The galaxy appears to be a fairly massive system with intermediate star formation activity.
