The object appears to be a galaxy with a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears somewhat spherical in shape. The galaxy displays a yellowish-orange color, suggesting a stellar population dominated by older, redder stars, and a reduced amount of on-going star formation. There is little evidence of spiral arm structure or prominent dust lanes. Overall, the galaxy presents a largely undisturbed structure, lacking strong signs of recent major merger events. The lack of visible features indicates a substantial fraction of the light emitted is from an evolved stellar population.
