The galaxy appears to be an elliptical galaxy, exhibiting a smooth, largely featureless morphology. Its shape is generally round. The galaxy possesses a bright, concentrated central bulge with a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy fade gradually into the background sky, with a subtle, diffuse halo. There is very little evidence of spiral arm structure or dust lanes. There do not appear to be any major disturbances or signs of merging activity. There are some faint blueish regions detected, perhaps signifying recent star formation.
