The galaxy presents as a somewhat elliptical structure, though it is not perfectly symmetrical, appearing slightly elongated in shape. Its overall color profile tends towards the redder end of the spectrum, suggesting a population of older stars with lower rates of star formation. There's a suggestion of interaction with a neighboring galaxy, as indicated by a visual distortion. The galaxy exhibits a relatively smooth texture. There are subtle irregularities in its luminosity distribution, possibly indicative of past or ongoing minor disturbances. The estimated mass of the galaxy is substantial, suggesting it's a mature system.
