This galaxy presents an elongated, cigar-shaped morphology. The light distribution appears relatively smooth, with no distinct spiral arms or bar structures discernible. The dominant color is a yellowish-orange hue, suggesting a population of older stars. It shows weak evidence of interaction or minor disturbances, possibly tidal features resulting from a past or ongoing gravitational interaction with the nearby object, but there is no clear merging. The half-light radius indicates a moderately sized galaxy. Overall, this galaxy appears to be a relatively evolved system.
