This galaxy presents a largely elliptical morphology, appearing quite smooth and centrally concentrated. The light profile suggests a spheroid-dominated system with minimal apparent disk structure. The galaxy's core region exhibits a bright, yellowish-orange hue, potentially indicating an older stellar population. This color transitions to a slightly greener color further away from the core. There may be indications of a minor tidal disturbance in the galaxy's outer halo, or potentially an ongoing minor merger event, contributing to the subtle irregularities in its shape.
