This galaxy exhibits a primarily smooth morphology, appearing as an elongated, cigar-shaped structure. The central region displays a concentration of light, suggesting a prominent galactic bulge. Moving outwards from the center, the galaxy appears to transition to a bluer hue. This may indicate the presence of a younger stellar population in the outer regions. There is some indication of minor disturbances in the galaxy's form, but it does not appear to be undergoing a major merging event. Another smaller object can be seen to the side of this galaxy, perhaps another smaller galaxy undergoing some sort of interaction. Overall, the galaxy seems to be fairly isolated and not heavily distorted.