The galaxy presents an overall elliptical morphology, with a relatively smooth, centrally concentrated light distribution. The core region exhibits a pronounced yellowish-orange hue, suggesting an older stellar population likely dominated by evolved red giant stars. Moving outward from the center, a faint, bluer component is visible, indicating the presence of some younger, hotter stars or potentially a low level of ongoing star formation activity. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. A slight asymmetry in the outer regions hints at a possible minor interaction or past accretion event. The disk component appears weakly defined, with a significant smooth component. No prominent dust lanes or spiral arm structures are discernible within the observed image. The redshift is low, and overall it is of moderate size.
