The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears somewhat elliptical, trending toward round, but without a clearly defined disk structure. The core region exhibits a yellowish hue, possibly indicative of an older stellar population. There are hints of fainter, bluer regions extending outwards, which may suggest some ongoing star formation. Morphological disturbances are subtle, but there's an indication of a possible minor interaction or merger event in its recent history based on the slight asymmetries detected in the outer regions of the galaxy. The overall color suggests a moderate level of star formation activity but is potentially dominated by an older stellar population.
