The observed galaxy presents as a centrally concentrated luminous object. It appears predominantly smooth in texture, with a near-spherical morphology. There is a notable absence of spiral arm structures or significant dust lane features. The light distribution appears quite uniform, diminishing gradually from a bright core outwards. The colour profile exhibits a yellow-orange hue, suggesting a population of older stars. Evidence of any tidal interactions or ongoing mergers is not readily apparent, although there might be hints of minor disturbances. Based on the estimated size, it appears to be a medium-sized galaxy. Overall, the visual characteristics suggest that this is likely an elliptical galaxy with an evolved stellar population and low star formation rate.
