The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, approaching a circular shape. The color profile suggests a dominant population of older stars, with a yellowish hue concentrated towards the core. There is little evidence of spiral arm structure or significant dust lanes. No obvious signs of ongoing major mergers are visible. There may be some minor asymmetry or faint features that suggest minor disturbances. Overall, the galaxy presents a quiescent appearance, potentially indicative of low star formation activity. The effective radius appears small, suggesting a compact structure.
