The galaxy presents a distinctly elongated, cigar-like morphology. Its color profile suggests an older stellar population, with a dominant yellowish-orange hue concentrated towards the central region, likely indicative of a galactic bulge. The galaxy exhibits a smooth texture, showing a lack of prominent spiral arm structures or significant dust lanes. There is a possible small disturbance or merger remnant near the center, indicated by a knot of slightly bluer light, suggesting a potential region of more recent star formation activity. Overall, this galaxy appears to be a relatively quiescent system, likely an elliptical or lenticular galaxy undergoing minimal current star formation.