The galaxy presents as a generally smooth object, with an elongated, cigar-like shape. It exhibits a color gradient, appearing more yellow-orange towards the center, suggestive of an older stellar population and potentially a higher concentration of dust. Fainter, bluer hues are observed towards the outer edges, possibly indicating regions of more recent star formation, although these features are not sharply defined. No obvious spiral arms or strong tidal features are apparent. The galaxy appears relatively isolated, with no immediate signs of ongoing major mergers or significant gravitational disturbances. The overall structure points towards a galaxy dominated by an evolved stellar population with a moderate amount of on-going star formation.
