The galaxy presents as a moderately luminous, elliptical morphology. It displays a relatively smooth light distribution, with a bright, concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. Surrounding this central region is a fainter, bluer halo, potentially indicating the presence of more recent star formation or a younger stellar population. The overall shape is somewhat elongated, but it's primarily rounded. No prominent spiral arms, bars, or tidal features are discernible, implying a lack of recent major merger events or significant gravitational disturbances. The galaxy seems fairly isolated and undisturbed, with a possible weak active galactic nucleus.
