The galaxy presents a morphology that is predominantly smooth in appearance, with a noticeable central bulge that appears slightly elongated. The core exhibits a yellowish hue, suggestive of an older stellar population. There is a faint, diffuse disk component surrounding the bulge, displaying a bluer color, which may indicate regions of ongoing star formation. Although the galaxy lacks distinct spiral arms, subtle irregularities in the outer regions hint at possible past or ongoing interactions. It's overall shape is somewhere between round and elliptical, with a hint of a cigar-like shape. There is no clear evidence of a major merging event, although minor disturbances cannot be ruled out.
