The galaxy presents as a luminous object with a dominant red hue, indicative of an older stellar population and/or significant dust attenuation. Its morphology appears to be generally smooth, with a suggestion of a disk-like structure. There is no clear evidence of prominent spiral arms. The galaxy is elongated, displaying a cigar shape. There are no signs of major mergers or significant tidal disturbances. Overall, this galaxy appears to be a relatively massive, passively evolving system.
