The galaxy presents as a single, moderately luminous object, exhibiting a generally elliptical morphology. The light distribution appears relatively smooth and concentrated towards the center, indicative of a high degree of radial symmetry. The galaxy’s color index suggests a population of older stars, potentially with ongoing, but relatively low, levels of star formation. There is a slight elongation along one axis, but no distinct spiral arm structure or prominent dust lanes are discernible. There are no obvious signs of tidal disturbances or interactions with other galaxies, suggesting a relatively isolated system or a past merger event that has reached a settled state. 
