The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, featureless morphology. The central region shows a high concentration of light, indicative of a prominent bulge. The luminosity decreases gradually towards the outer regions, with no distinct spiral arms or disk-like structures visible. The galaxy's overall shape is elongated, suggesting a moderate degree of ellipticity, falling somewhere between round and cigar-shaped. There is little evidence of ongoing mergers or significant tidal disturbances based on this image. A slight color gradient is observed, where the core region appears more reddish, possibly indicating an older stellar population. The galaxy's peripheral areas show bluer hues, potentially revealing the presence of younger stars.
