This galaxy exhibits a primarily smooth morphology, appearing as a somewhat elongated, cigar-shaped structure. There are hints of a disk-like component, though the overall light distribution is dominated by a central bulge or spheroid. The color gradients suggest a centrally concentrated population of older stars, appearing reddish, with a bluer, potentially younger stellar population distributed throughout the more extended disk. The galaxy does not show any strong signs of recent major merger activity, though a possible minor disturbance in the form of a slight asymmetry could be present. Given the lack of distinct spiral arms or significant dust lanes, it appears to be an early-type disk galaxy or possibly a lenticular galaxy viewed edge-on. The size of the galaxy is relatively compact, and the estimated star formation rate appears quite low. The estimated stellar mass is moderate, suggesting a galaxy of intermediate size and luminosity.
