The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge. The galaxy appears nearly round with a slight ellipticity. No distinct spiral arms or prominent dust lanes are discernible. The color is generally consistent across the visible portion of the galaxy, suggesting a relatively homogenous stellar population. The galaxy appears to be undisturbed, showing no major signs of mergers or tidal interactions. Faint extensions or minor disturbances may be present, but they do not significantly alter the overall smooth appearance. The luminosity suggests a moderate size. The lack of prominent blue regions indicates a low rate of active star formation. The galaxy likely consists primarily of older, redder stars.
