The galaxy appears to be a relatively smooth, elliptical type, exhibiting a centrally concentrated light profile. The core is luminous with a yellowish hue, likely indicating an older stellar population. The luminosity gradually decreases towards the outer regions of the galaxy. The shape is slightly elongated, but overall close to round. There are no distinct spiral arms or prominent dust lanes visible. The galaxy does not appear to be undergoing a major merging event, although some minor disturbances may be present. The outer regions show a slight blue tinge, possibly indicating some level of recent star formation, albeit at a relatively low rate. Overall, the galaxy presents as a mature, massive system, with a significant spheroidal component.
