The galaxy presents as an elliptical morphology, appearing somewhat smooth and centrally concentrated. The core exhibits a yellowish-white hue, likely indicative of an older stellar population. Fainter, diffuse bluish regions are observed extending outward from the core region, possibly representing areas of more recent, though not vigorous, star formation. A subtle disk-like feature may be present, though not prominent, oriented approximately horizontally across the image. There may be some evidence of minor disturbances within the galaxy's structure, perhaps hinting at a past or ongoing minor interaction or merger. Overall, the galaxy appears relatively isolated and undisturbed.
