The galaxy presents as a relatively smooth, centrally concentrated object, suggesting an elliptical morphology. The overall color profile appears to be indicative of an older stellar population, with a yellow-red hue dominating the light output. There are no visible spiral arms or dust lanes, further supporting the elliptical classification. The light distribution is highly concentrated towards the center. There are no apparent signs of recent or ongoing major mergers or tidal disturbances. The galaxy does not appear to be perfectly circular but presents some ellipticity with its major axis oriented approximately Northwest to Southeast.
