The galaxy appears as a relatively smooth, elliptical object with a concentrated central bulge. There is a lack of distinct spiral arm structure, and it appears largely featureless. The color gradient suggests an older stellar population with a dominant yellow/red hue in the central region, likely indicative of evolved stars. The outer regions show a subtle blue tinge, potentially hinting at ongoing, albeit subdued, star formation. The overall shape is neither perfectly spherical nor highly elongated; it is somewhere in between. There is no obvious evidence of any major merger events or significant tidal disturbances affecting the morphology of the galaxy. Any ongoing star formation is at a low rate.
