The galaxy presents a largely smooth, elliptical morphology with a dominant central bulge. The light distribution is relatively even, lacking prominent spiral arms or significant dust lanes. There is an indication of a secondary, slightly smaller, structure superimposed above.

The color profile suggests an older stellar population, with a reddish-orange hue predominating. This implies a relatively low rate of ongoing star formation within the galaxy at the current epoch. There might be a very low level of star formation occurring, especially within the bulge and secondary structure. The overall shape of the galaxy is generally round, with minimal elongation. There is some visual evidence to support a possible merger event. The object displays little evidence of a significant tidal disruption.
