Observed galaxy presents an overall elliptical morphology with a concentrated central bulge. The luminosity profile indicates a significant concentration of light towards the center. There appears to be some disk structure, with a faint, diffuse extension around the bulge. The galaxy exhibits color variation, with a slightly bluer region visible in the central area transitioning to redder hues on the edges.

There are potential indications of minor disturbance in the overall morphology, though the primary structure remains generally coherent. Some irregularities or faint tidal features could suggest a recent or ongoing minor interaction with another galaxy. Evidence of an active galactic nucleus is not apparent.
