The galaxy presents a predominantly smooth morphology, exhibiting characteristics suggestive of an elliptical or lenticular type. The central region is a concentrated luminosity, potentially indicating a substantial galactic nucleus. Moving outward, the light gradually diffuses, but overall still exhibiting a fairly symmetrical shape. Some subtle irregularities and minor distortions can be observed, hinting at either ongoing or past interaction or merger events. There appears to be a weak disk-like feature, but the prominence is quite low and this might be due to slight distortions in its profile. Coloration suggests a mixed stellar population, with regions of both older, redder stars and areas that could contain younger, bluer stars.
