The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a predominantly smooth, featureless morphology. It is elongated in shape, with a cigar-like appearance, and a high degree of central concentration. There is little to no visible structure suggestive of spiral arms or a prominent disk. The color gradient indicates a generally older stellar population, with the central region exhibiting a slightly redder hue compared to the outer regions which have a bluer color. No significant signs of recent or ongoing mergers or major disturbances are observed, although there may be some minor disturbances present. Based on the general color and shape, a classification towards the red sequence of galaxies seems likely.
