The galaxy presents an elliptical morphology, appearing largely smooth and relatively featureless. The color profile is dominated by warmer tones in the central region, suggesting an older stellar population. There appears to be minimal evidence of spiral arm structure or significant dust lanes. The overall shape is generally round, with only a slight deviation towards elongation. There are indications of possible minor disturbances in the galaxy's structure, but there are no clear signs of ongoing major merging activity or significant tidal distortions.
