The galaxy appears as a concentrated, elliptical-like structure with a smooth, diffuse profile. The central region exhibits a higher concentration of light, appearing a bright yellowish-orange, with the intensity gradually decreasing towards the outer regions. There is a subtle color gradient noticeable, where the central region has a slightly warmer hue.

The galaxy seems to have minimal visible substructure or spiral arm features, giving the impression of a relatively evolved system. There may be a faint suggestion of a disk, but it is not well-defined. The morphology suggests a classification towards the early-type end of the Hubble sequence, with the light being dominated by an older stellar population. There does not appear to be evidence of active merging or significant tidal disturbances, with an undisturbed structure.
