The galaxy presents as a relatively smooth, elliptical morphology. Its structure is dominated by a central bulge, appearing as a concentrated, bright region. There is limited evidence of spiral arms or distinct disk features. The galaxy appears to be a spheroid, with a mostly even luminosity profile that decreases radially. There appears to be some slight disruption to the galaxy's form, but not significant. The galaxy exhibits a color gradient, appearing bluer towards the center, suggesting the presence of younger stellar populations, and redder towards the edges, which may be indicative of older stars.
