The galaxy presents an elongated, cigar-shaped morphology. It displays a smooth appearance with a concentrated central bulge, suggesting an evolved stellar population. The color profile indicates a predominantly older stellar population, with a yellow-red hue dominating the central region. Fainter, bluer regions are visible in the outer extents of the galaxy, potentially indicating areas of on-going, albeit subdued, star formation. There is no apparent major disturbance or signs of an ongoing merger event, though a slight asymmetry in the outer regions hints at a possible minor interaction in the past. Overall, the galaxy appears as a relatively massive, quiescent system.
