The galaxy presents an elongated, cigar-shaped morphology. Its light profile appears relatively smooth, with a concentrated central region. There is a slight gradient in color across the galaxy, with the core exhibiting a subtly redder hue compared to the slightly bluer, outer regions. There are no strong indications of spiral arm structure. The overall smooth appearance suggests a system dominated by an older stellar population, although subtle color variations indicate ongoing, yet relatively subdued, star formation activity. There is no evidence of major mergers or significant tidal disturbances in the galaxy's structure.
