The galaxy presents a generally smooth and concentrated morphology. It exhibits a bright, centrally concentrated core that gradually fades towards its outer regions. The overall shape appears to be elliptical, with the galaxy exhibiting a moderate degree of roundness. There is no evidence of prominent spiral arms or a well-defined disk structure. The galaxy's color profile suggests a relatively evolved stellar population, with a yellowish hue indicating the presence of older, redder stars. There is a lack of discernible dust lanes or active star-forming regions within the galaxy. No signs of major disturbances, such as tidal tails or disrupted structures, indicating that the galaxy is likely undisturbed and not currently undergoing a major merger event. Faint hints of extended diffuse light are visible, possibly a halo of older stars surrounding the main body of the galaxy.
