The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which appears nearly spherical in projection. The light distribution is generally even, with a gradual decline in intensity moving outward from the core. Faint extensions appear to be present, giving it an overall somewhat oblong shape. There's no obvious spiral arm structure visible. The color gradient suggests older stellar populations are dominant within the galaxy, with a higher concentration of redder colors towards the core. The morphology indicates the galaxy is not undergoing any major merging activity or significant tidal disturbances.
