The galaxy presents as a relatively compact object. It appears to be largely spheroidal, exhibiting a smooth and fairly uniform distribution of light across its body, with little to no indication of spiral arms or other distinct features. The color profile suggests a population of older stars, leaning towards the redder end of the spectrum, which is consistent with a low rate of ongoing star formation. The overall morphology is suggestive of an elliptical galaxy in the early to mid stages of its evolutionary timeline. There appears to be some blue light towards the center, indicating some star formation. There may be some minor disturbances in the structure, but the overall roundness indicates no mergers are present.
