The galaxy presents a largely featureless morphology, exhibiting a smooth light distribution. It appears elliptical or spheroidal in shape, with an intermediate axis ratio. The concentration of light is highest towards the galactic center, gradually decreasing towards the outer regions. The dominant color is a yellowish hue, suggesting a population of older stars. No distinct spiral arms or prominent dust lanes are discernible. There is no evidence of tidal tails or other major morphological disturbances, indicating that the galaxy is likely not undergoing a major merger event. Faint, diffuse light extends some distance beyond the bright central region, giving the galaxy a relatively large apparent size.
