The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. Its overall shape appears elongated, with a cigar-like appearance. There is minimal visual evidence of spiral arms or a distinct disk. The light distribution is fairly even, with a gradual decline in brightness from the core outwards, indicative of an older stellar population and reduced star formation. There is no clear indication of a recent or ongoing major merger event, though a minor disturbance cannot be ruled out. The galaxy exhibits a reddish hue, suggestive of a population dominated by evolved stars.
