This galaxy exhibits a generally elliptical morphology, appearing somewhat compact. The central region is bright, displaying a concentrated luminosity profile. A slight blue tint is observed within this core, possibly indicative of a population of younger, hotter stars.

Moving outward from the center, a fainter, more diffuse halo is observed. This halo seems to extend further along the horizontal axis than the vertical, contributing to the elliptical shape. There is a slight hint of a possible disturbance to the bottom right of the core that causes the edge to seem less sharp.

Overall, the galaxy appears to be relatively isolated and does not show any obvious signs of interaction with other galaxies, with the caveat that some disruption may be present on the outskirts of the galaxy. The presence of a smooth profile suggests the galaxy is likely an early-type, potentially an elliptical or lenticular galaxy.
