The galaxy presents as a relatively smooth, centralized object. It has a largely elliptical morphology with a slightly elongated shape. The light profile appears centrally concentrated with a bright, somewhat diffused core, suggesting a possible bulge component. Surrounding the core is a fainter, more extended halo or disk. The color profile is mostly uniform across the galaxy with a somewhat blue-green hue in the outer regions, potentially indicating ongoing, though weak, star formation. There is no evidence of strong spiral arm structure or a prominent dust lane. The overall appearance is largely undisturbed and doesn't show signs of a major ongoing or recent merger event. Faint asymmetric features are visible, suggesting the possibility of a minor tidal interaction or disturbance. The effective radius is about 4 kpc. The estimated redshift places it at a distance where the light from younger stars would be visible, though the galaxy is not particularly luminous.
