The galaxy presents as a relatively smooth, elliptical morphology, with an apparent lack of significant spiral arm structures or prominent dust lanes. The central bulge is bright and dominant, indicating a likely high concentration of stars. The light distribution decreases gradually from the center outwards, suggesting a centrally concentrated stellar population. The galaxy's overall color appears to be skewed towards the redder end of the spectrum, hinting at an older stellar population and reduced on-going star formation. There are no obvious signs of recent major merger events or significant tidal disturbances. There is a slight disk component.