The galaxy presents a generally smooth appearance, with a discernible elliptical shape. The color distribution indicates a bulge with a redder hue, potentially indicating an older stellar population. Moving outward from the bulge, the galaxy displays a transition to slightly bluer tones, suggesting the presence of younger, hotter stars in the outer regions. The overall morphology is consistent with that of an early-type galaxy. There's a slight asymmetry or a subtle feature that may suggest a minor gravitational interaction in its past, or potentially a faint, disturbed disk component. The galaxy displays a moderate size and luminosity. Overall, the galaxy appears to be relatively isolated and doesn't show any significant signs of ongoing major mergers or significant disturbances.
