The galaxy presents an elongated, cigar-shaped morphology. Its light distribution appears relatively smooth, with some indication of a possible disk-like structure, though detailed features are not readily discernible. The galaxy exhibits a yellowish-orange hue, suggestive of an older stellar population. There is no obvious central bulge, or spiral arms, and the galaxy appears to be largely undisturbed, showing no prominent signs of ongoing merger activity or significant tidal disruptions. Overall, the galaxy appears to be a moderately massive system with a relatively low specific star formation rate.