The galaxy presents as a centrally concentrated object, likely a spheroid. It exhibits a relatively smooth morphology with a mostly homogenous distribution of light across its structure. The galaxy shows a slightly elliptical shape, although approaching circular, with no discernable spiral arm structure.

The color profile suggests a dominant population of older stars, as indicated by the presence of redder hues. The lack of intense blue regions suggests a low rate of ongoing star formation activity within the galaxy. There are some irregularities to its structure. A possible merging event appears to be occurring in this galaxy, with multiple nuclei visible. There is a tidal tail visible above the nuclei, indicating past or ongoing interaction with another galaxy. 
