The galaxy presents as a generally smooth, elliptical object. Its core is a bright, concentrated yellow, suggesting a population of older stars. There is a slight asymmetry to the overall shape, with a hint of a flattened disk-like structure, or perhaps a minor tidal disturbance. The outer regions fade into a bluer hue, possibly indicating some degree of ongoing, though subdued, star formation in the outer regions. The galaxy exhibits a moderate size, neither particularly large nor especially compact. There may be some evidence of minor interaction or a past merger event, given the deviation from a perfectly smooth profile and the slightly irregular light distribution in the outer regions. The elongated shape is much more likely of an elliptical galaxy, though the slight flattening and faint bluer regions hint at a possible disk component. 
