The galaxy presents as a largely featureless, elliptical form. The central region displays a high concentration of luminosity, exhibiting a bright, yellowish-white core that diminishes in intensity towards the outer edges. The overall color profile suggests a relatively older stellar population, with a dominance of redder wavelengths. There is no evidence of prominent spiral arms, dust lanes, or active star-forming regions. The galaxy appears to be relatively isolated, without any obvious signs of tidal interactions or ongoing mergers, though a mild disturbance is possible. It is moderately rounded. The estimated size is around 6.6 Kpc. It has an estimated mass of around 10^11 solar masses and a low star formation rate.
