The galaxy appears to be an elliptical type, exhibiting a generally smooth, concentrated morphology with little to no discernible spiral arm structure. Its shape is predominantly round, though a slight ellipticity is noted. The galaxy displays a yellowish-orange hue, indicating an older stellar population dominated by redder stars. This color suggests relatively low levels of ongoing star formation. There is no evidence of significant tidal disturbances or interactions with other galaxies, based on the absence of extended plumes or distorted features. The galaxy presents a well-defined central bulge. The light is somewhat diffuse, suggesting a gradual decline in stellar density from the core outwards.
