The galaxy presents as an elliptical type, exhibiting a smooth, relatively featureless morphology. Its shape appears nearly circular in projection. There is minimal evidence of ongoing merging activity or significant tidal disturbances. The galaxy shows a concentration of light towards the center, indicative of a substantial galactic nucleus or bulge. There appears to be a lack of distinct spiral arm structures or prominent dust lanes. Color gradients across the galaxy may suggest variations in stellar populations, with the central regions potentially hosting older, redder stars, and the outer regions possibly containing younger, bluer stars. Overall, the galaxy appears relatively quiescent and evolved.
