The galaxy presents as a relatively compact object with a smooth, elliptical morphology. It exhibits a fairly homogenous luminosity profile across its body, with no distinct central bulge or spiral arm structure discernable. There are no obvious dust lanes or patches of intense star formation visible in this imaging, suggesting a lack of significant recent star formation activity. The overall color appears moderately red, indicative of an older stellar population dominating the galaxy's light output. The galaxy appears to be isolated and unperturbed, showing no signs of ongoing merger activity or tidal interactions with nearby galaxies.
