The galaxy presents as a relatively smooth, elongated structure with a noticeable bulge. Its apparent shape is cigar-like, indicating an elliptical morphology or a disk galaxy viewed at a steep inclination. The light distribution suggests a centrally concentrated luminosity profile, diminishing towards the edges. The galaxy exhibits a color gradient; the core appears to be of a yellower hue, possibly indicative of an older stellar population. The outer regions show a subtle blue tint, which could indicate the presence of younger stars or regions of on-going star formation, albeit at a modest rate. There appears to be little to no evidence of prominent spiral arms or significant dust lanes based on the image's resolution. No tidal features or signs of recent major mergers are clearly visible, suggesting a generally undisturbed system, though minor disturbances cannot be entirely ruled out.
