The galaxy presents a smooth, elliptical morphology. The central region exhibits a concentrated, bright core with a yellow-orange hue, suggesting an older stellar population. A slight extension is observed, possibly indicating tidal interactions or minor disturbances. It may be merging with another smaller galaxy nearby, as indicated by the irregular shape and faint, bluish area on one side, with two separate centers of luminosity. This blue region suggests the presence of some younger, hotter stars within this merging galaxy. Overall, the system shows a blend of mature and possibly actively forming stellar populations with clear signs of gravitational interaction.
