The galaxy presents as a moderately luminous object at a redshift of approximately 0.095, indicating a substantial distance. Its morphology appears to be primarily smooth, with a suggestion of a disk-like structure viewed at a significant angle. The galaxy's shape is elongated, approaching a cigar-like form. There is no strong evidence of ongoing major mergers, although some minor disturbances cannot be ruled out. The color profile suggests a population dominated by older stars, contributing to its relatively redder appearance. The galaxy is likely to be quite massive, displaying a modest star formation rate.
