The galaxy presents a generally smooth and concentrated appearance, appearing mostly spheroidal in shape with an approximate effective radius of 6 kpc. The light profile is centrally concentrated, with a gradual decrease in brightness towards the outer regions. The galaxy exhibits a color gradient, appearing more yellow-white in the central region, shifting toward a redder hue at the edge of the galaxy, indicating a potential variation in stellar populations and/or dust content. There is a slight asymmetry to the galaxy's overall shape, however, it is fairly smooth. There is no evidence of strong spiral arm structures or a well-defined disk. Possible low-level star formation is observed. No distinct tidal features or merging companions are apparent in the immediate vicinity, which suggest a relatively isolated system, and that the galaxy is not currently undergoing a major merger event.
