The galaxy presents as a somewhat elliptical, though mostly round, structure with a diffuse glow. Its light distribution appears relatively smooth and concentrated, with a gradual fading towards the edges suggesting a lack of distinct spiral arms. The core appears brighter and slightly more compact than the outer regions. There are indications of a possible minor interaction or tidal disturbance based on faint distortions visible in the outer halo. The overall color of the galaxy appears to be yellowish-red, indicating an older stellar population and a relatively low rate of current star formation. There is no presence of very dusty regions.
