The galaxy presents as a somewhat elongated, disk-like structure, viewed at an oblique angle. It exhibits a smooth, featureless appearance with a noticeable central bulge that appears more concentrated and luminous. The color profile indicates a redder hue in the central region, possibly signifying an older stellar population, while the outer regions of the disk appear bluer, suggestive of ongoing or recent star formation. The galaxy's overall shape is cigar-like. There is no apparent evidence of strong tidal interactions, merging activity, or significant disturbances in its structure.
