This galaxy presents as a relatively smooth, elliptical structure. There is a concentration of light toward the center, suggesting a central bulge. No distinct spiral arms are observed, and the overall light distribution is fairly uniform. The galaxy exhibits a somewhat round shape, and there is no clear evidence of tidal tails or other distortions indicative of recent or ongoing merger activity. The color profile suggests a population of older stars. There are no discernible dust lanes or features indicative of active star formation within the visible portion of this galaxy.
