The galaxy presents a largely smooth and elliptical appearance. It exhibits a concentrated central bulge that transitions into a less defined halo. The core region displays a slight reddish hue, possibly indicative of an older stellar population. Extending outwards, a diffuse, bluish-greenish aura surrounds the central region, suggesting the presence of younger stars. There is no apparent spiral structure or bar feature within the galaxy's morphology. Faint, subtle disturbances or minor irregularities might be present in the outer regions but the quality of the image makes it difficult to assess. The overall impression is that of a galaxy undergoing passive evolution with relatively low levels of star formation. It appears to be in a fairly relaxed state, with no significant signs of ongoing mergers or major disturbances. The circular shape is fairly complete, with no noticeable skew.
