The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The light profile appears centrally peaked. A faint, diffuse halo extends outward from the brighter core, fading into the background. There are no obvious spiral arm structures or dust lanes visible. The galaxy appears generally rounded in shape with no significant distortions. The galaxy's color index indicates a population of older, redder stars dominating the luminosity output. Star formation appears to be low within the galaxy, possibly nearing quiescence. There are no indications of recent or ongoing merger activity, suggesting a gravitationally relaxed state.
