The galaxy presents as a generally smooth, elliptical-like object with a moderate degree of elongation. There's a central concentration of light, with a gradual decrease in luminosity extending outwards. The color profile appears to consist of a mix of blue and redder hues, with the central region showing a pinkish tint, potentially indicative of a mix of stellar populations. No prominent spiral arms or distinct features are immediately apparent. Based on its color and smooth morphology, this galaxy likely consists of older stars. There is no significant evidence of a major ongoing merger event, but minor disturbances are possible.
