The galaxy presents an elongated, cigar-like morphology. It appears relatively smooth with a gradual increase in intensity towards the center, suggesting a centrally concentrated stellar population. The overall color profile is indicative of a mixed population of stars, with a subtle bluer hue most likely due to star formation, but overall is redder suggesting older stars. No spiral arm structures are clearly visible. There is no evidence of significant tidal disturbances or ongoing major mergers; however, minor disturbances cannot be fully ruled out at this resolution.
