The galaxy presents as an elongated, cigar-shaped form, appearing largely smooth with a concentrated central bulge. The color profile indicates a redder hue in the central region, possibly indicative of an older stellar population. Fainter blue tinges are observed towards the outer edges of the galaxy, suggesting some ongoing or recent star formation, albeit at a modest level. No spiral arm structures or prominent dust lanes are clearly discernible. The overall appearance suggests a system in a relatively advanced stage of evolution, leaning toward an elliptical morphology but retaining some residual disk-like characteristics. There might be some minor gravitational disturbance or interaction evidenced by the slight asymmetry in its outer regions.
