The galaxy appears to be a relatively small elliptical galaxy. It exhibits a smooth, centrally concentrated light distribution with a slight elongation, suggesting a possible oblate spheroid shape. The core of the galaxy presents a brighter, more intense luminosity compared to the outer regions. There's a very subtle disk feature within it. The color profile of the galaxy indicates an older stellar population, with the redder hues dominating the color profile. Evidence of recent or ongoing star formation is minimal, indicated by the overall passive nature and lack of prominent blue regions typically associated with younger, hotter stars. The galaxy does not appear to be undergoing any major merging events.
