The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its color gradient indicates an older stellar population, with a yellowish-orange hue dominating the central regions, suggesting a lack of ongoing significant star formation. The galaxy exhibits a slight elongation, tending towards a cigar shape, but is largely categorized as in-between round and elongated. No prominent spiral arm structures or significant dust lanes are discernible. The overall appearance suggests a mature galaxy that has largely exhausted its gas supply. There is no visual evidence of any major merging activity or significant tidal disturbances in its immediate vicinity. Minor disturbances, such as subtle asymmetries in the light distribution, cannot be entirely ruled out. The galaxy's smooth appearance and the absence of significant star formation activity are consistent with it residing on the red sequence.
