The galaxy presents a generally smooth morphology, exhibiting a concentrated central bulge with a subtle extension that may hint at a nascent or disrupted disk structure. The light distribution is largely uniform, suggesting a lack of prominent spiral arms or distinct star-forming regions. The object is slightly elliptical with a color index suggesting a population of older stars. There is no evidence of a major ongoing merger, although there may be a slight disturbance of the galaxy's overall shape. Given its apparent magnitude and redshift, this galaxy is intrinsically luminous.
