This galaxy exhibits an elliptical morphology, displaying a smooth and concentrated light profile. The galaxy appears slightly elongated, deviating moderately from a perfectly circular shape. The central region shows a high concentration of light, suggesting the presence of an older stellar population. The galaxy exhibits a redder hue centrally with a subtle shift towards bluer tones in the outer regions. There is little evidence of spiral arms, dust lanes, or significant star formation activity from the color and lack of distinct features. There does not appear to be any significant interaction or merging activity affecting the overall structure of the galaxy based on visual inspection. The light appears fairly symmetrical indicating that it is not highly disturbed. Overall, this appears to be an elliptical galaxy, with little to no observable features and an older stellar population.
