The galaxy presents a generally elliptical morphology, appearing largely smooth and concentrated towards its center. The light profile shows a strong central bulge region that is predominantly yellow. This suggests a relatively older stellar population dominating the core, indicating a lower rate of on-going star formation. Fainter, more diffuse light extends outwards from the central bulge, gradually fading into the background. No distinct spiral arms or features indicative of recent major merging events are readily apparent. There may be only minor disturbances observed in the galaxy's outer regions. The object appears relatively isolated, further supporting the lack of recent major interactions.
