The galaxy presents a predominantly smooth, elliptical morphology. There is no distinct spiral arm structure visible. The light distribution appears highly concentrated toward the center, indicating a prominent bulge. The galaxy exhibits a generally round shape with minimal deviation from circularity. The color profile suggests an older stellar population with a yellowish-red hue, possibly indicating a lack of significant recent star formation. No signs of ongoing major mergers or significant tidal disturbances are readily apparent, suggesting a relatively quiescent evolutionary state.
