This galaxy exhibits an elongated, cigar-like morphology. The light distribution appears relatively smooth, with a concentration of older stars toward the central region, giving it a yellowish-orange hue. There is a slight hint of bluer light towards the edges of the galaxy, suggesting the presence of some younger stars, although the overall star formation rate appears to be relatively low. There is little visible evidence of strong tidal disturbances or a recent major merger event. A very small portion of the galaxy might be experiencing minor disturbances based on visual inspection, though further investigation is needed.