The galaxy presents a largely smooth, elliptical morphology. The light distribution is concentrated toward the center, exhibiting a bright, unresolved core that is indicative of an older stellar population. The galaxy appears to be relatively isolated, with no obvious signs of recent or ongoing major mergers or tidal disturbances. A slight color gradient is observable, transitioning from a yellowish hue at the center to a redder tint in the outer regions. This suggests a possible decline in recent star formation activity and increasing age of the stellar population towards the galaxy's outskirts. There are also hints of faint features or disks within it.
