The galaxy appears as a centrally concentrated object with a generally smooth profile. The central region displays a yellowish hue, indicative of an older stellar population. The galaxy exhibits a somewhat elliptical shape, but is relatively round. There is no significant evidence of spiral arm structure or a prominent disk component. The overall structure suggests minimal signs of recent major mergers or significant tidal disturbances, though there may be a slight asymmetry in the outer regions. This galaxy appears to be a relatively massive and luminous object, exhibiting a low star formation rate.
