The galaxy presents as an elliptical or spheroidal system, exhibiting a high degree of smoothness in its overall morphology. There is a distinct central bulge that gradually fades outward. The isophotes appear largely round, indicating a low degree of ellipticity. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy does not appear to be undergoing any major merging activity or tidal disturbances. The color profile suggests a stellar population with a relatively low rate of star formation, leaning toward an older, redder population with less gas and dust. The estimated size of the galaxy is a few kiloparsecs in radius.
