The galaxy presents a generally smooth morphology. It appears largely featureless, with no obvious spiral arms or bar structures visible. Its overall shape is somewhat elliptical, exhibiting an elongation that places it somewhere between round and cigar-shaped. There is a suggestion of a central concentration of light, indicative of a possible bulge. The galaxy’s color appears to be trending towards the redder end of the spectrum, potentially indicating an older stellar population. There is a slight asymmetry in its overall structure, hinting at a minor gravitational interaction or disturbance. No tidal tails or other prominent signs of a major merger are immediately apparent.
