The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. Its overall shape is elliptical, appearing somewhere between circular and elongated, with a slight cigar-like appearance to it. The light profile suggests a higher concentration of older stars, indicated by the yellowish hue in the central region, gradually fading into a redder outer halo. There is no discernible structure of spiral arms or a prominent disk component. No tidal tails or signs of recent major merger events are visible. Subtle disturbances may exist within the faint outer halo. The overall appearance indicates the galaxy is most likely an elliptical galaxy, potentially undergoing minor interactions.
