The galaxy presents as a relatively compact, well-defined elliptical structure. Its morphology appears largely smooth, with a high degree of central concentration and a generally spheroidal shape, presenting an even distribution of light across its surface. There is no evidence of prominent spiral arms, bars, or other distinct features characteristic of disk galaxies. The galaxy appears to be isolated, with no readily apparent signs of tidal interactions or ongoing merger activity. Its light is redder than average in color, hinting to an older stellar population.

