The galaxy presents as a fairly smooth, elliptical structure. The light distribution suggests a centrally concentrated bulge with a noticeable falloff in luminosity towards the outer regions. There appears to be little evidence of distinct spiral arms or significant dust lanes. The object appears to be more elongated than perfectly circular, leaning towards a slightly cigar-like shape. The color gradient suggests an older stellar population dominating the central region, as indicated by the yellower hue. Hints of bluer light towards the periphery imply the presence of younger, star-forming regions, though they are not particularly prominent. There isn't a discernible indication of tidal features or major morphological disturbances, suggesting the galaxy is relatively isolated and undisturbed. Faint asymmetric features on one side could indicate a minor interaction or recent minor merger.
