The galaxy presents a primarily smooth, elliptical morphology, with a concentrated central bulge exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions display a fainter, somewhat more diffuse glow, with hints of reddish areas perhaps indicative of some recent, albeit limited, star formation.  The galaxy's overall shape appears elongated, but not significantly so, tending towards a more intermediate elliptical form. There is some evidence of minor disturbance to the upper left, but it is not immediately clear if this is a result of a merger, tidal interaction, or internal activity. The galaxy exhibits an estimated diameter in the tens of thousands of light years.
