The galaxy exhibits a generally smooth morphology. Its shape appears largely round, with minimal deviation towards an elongated or cigar-like form. There's no strong evidence of a prominent disk structure or spiral arms. The color profile is dominated by redder hues, but has hints of green around the central region, indicating the possibility of some active star formation. The presence of red and a lack of blue indicates a mostly older stellar population and the lack of ongoing major star formation. A small region in the center has a pink hue which could point to the presence of ionized gas, which can often indicate active galactic nuclei. There are no immediately apparent signs of significant ongoing merging activity, though subtle irregularities in its overall form suggest the possibility of minor past interactions or disturbances. A close visual inspection suggests the galaxy is likely an elliptical type or a lenticular type with a smooth profile and little to no spiral structure.
