The galaxy appears as a relatively smooth, elliptical-like structure. Its color gradient transitions smoothly from a bright, yellowish-white center to a dimmer, bluish outer region, suggesting a decreasing concentration of older stars towards the periphery. There is no clear evidence of spiral arms, a bar, or significant dust lanes. The galaxy presents with intermediate roundness, appearing somewhat circular, without elongation into a cigar shape. The galaxy appears undisturbed, without any obvious signs of merging or major interactions. The low star formation rate is consistent with its apparent morphology, further suggesting a relatively evolved system dominated by an older stellar population.
