The galaxy presents as a relatively smooth, elliptical-like object. It exhibits a centrally concentrated light profile, appearing brightest in the core region with a gradual decrease in luminosity outwards. There is a slight elongation, but the overall form is largely rounded.  The galaxy displays a generally uniform color across its body with some variation in hues. There is an absence of prominent spiral arms, dust lanes, or distinct morphological features associated with active star formation. No significant signs of tidal disturbances or mergers are readily apparent. The galaxy appears to be relatively isolated in its immediate vicinity. The color index appears to be redder compared to typical spiral galaxies, suggesting an older stellar population and reduced recent star formation activity.
