The galaxy presents as a somewhat smooth, oblate spheroid. The central region is a bright, yellowish-white color, indicating an older stellar population or significant dust obscuration. There is a subtle redder region visible on the left side of the galaxy, potentially indicative of ongoing, albeit low-level, star formation or a localized dust lane. The outer regions show a subtle gradient towards a bluer hue, which may be related to increased star formation in the outskirts. There appears to be some minor disturbance or possible interaction occurring. The galaxy is not perfectly symmetrical, suggesting it is not a relaxed system. Overall, the morphology suggests a galaxy in transition, possibly evolving from a disk galaxy into a more elliptical shape, or that has undergone a merger event in the relatively recent past.
