The galaxy presents as a relatively smooth, elliptical structure with a cigar-shaped morphology. It exhibits a noticeable color gradient, transitioning from a bluer hue in the central regions to redder tones towards the periphery. This may indicate an older stellar population dominating the outer regions, with ongoing or recent star formation possibly concentrated towards the center, though the overall star formation rate appears to be low. There is little evidence of spiral arm structure or a prominent disk. The galaxy appears relatively isolated, showing no signs of major interactions or mergers. The presence of minor disturbances is not completely ruled out, but it's likely that this galaxy is primarily evolving in isolation. The size of the galaxy appears modest compared to other galaxies, indicating it is a dwarf galaxy.
