The galaxy presents a roughly elliptical morphology, with a high degree of central concentration. The primary body of the galaxy exhibits a smooth, luminous profile, with no readily apparent spiral arm structure. The color gradient shifts from a central yellowish hue to a bluer tint in one section. This bluer region suggests more recent star formation activity or a distinct stellar population. The galaxy's overall structure appears disturbed, indicating a possible interaction or merger event. There are no clear tidal tails or extended halo structures visible in this image. The object suggests a relatively relaxed system dominated by older stellar populations. However, the slight asymmetry and the localized blue region suggest the presence of ongoing or recent interactions. 
