The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core region exhibits a yellow-orange hue, possibly indicative of an older stellar population dominating in this area. Surrounding the core is a fainter, more diffuse halo, which has a slightly blue-green tint. This may signify the presence of younger, hotter stars or ongoing star formation activity, although at a relatively low rate. The overall shape appears somewhat elliptical with a ratio of about 2:1 for major to minor axis. There is no strong evidence of spiral arms or a well-defined disk structure in this image. No signs of any major merger events or significant tidal disturbances are observable. The galaxy exhibits an overall lenticular-like appearance.
