The galaxy presents as an elongated, disk-like structure with an apparent cigar shape, suggesting an elliptical morphology. The luminous profile appears relatively smooth, with a concentrated central bulge exhibiting a yellowish-white color indicative of an older stellar population. Faint disk-like structures, with a bluer hue, suggest a low level of ongoing star formation. There is no evidence of major mergers or strong tidal features. The overall appearance implies an evolved system with a dominant spheroidal component.