The galaxy presents a primarily smooth morphology, with an overall elliptical shape. The central region exhibits a concentrated, bright, yellowish hue, suggesting a population of older stars. Fainter, bluer light extends outward from the core, possibly indicating some regions of active star formation. Slight asymmetry or a minor disturbance is visible in the outer regions, which could be evidence of tidal interactions or a recent minor merger event. There may be faint, diffuse extensions on opposing sides, possibly indicative of tidal tails, though not prominent.
