The galaxy appears as a slightly elongated, diffuse object with a smooth morphology. The light distribution is concentrated towards the center, suggesting a significant bulge component. The color profile indicates the presence of older stellar populations, giving it a reddish hue. There may be subtle irregularities or faint features extending from the main body, suggesting potential minor disturbances or interactions. The overall shape is somewhat intermediate between round and elongated. The galaxy does not show strong evidence of spiral arms or active star formation.
