The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile with a noticeable central bulge. The galaxy's overall shape is somewhat elongated, leaning toward an intermediate elliptical classification. The light distribution suggests a relatively old stellar population, characterized by a yellowish hue in the central regions, indicative of evolved stars. There are hints of a faint, diffuse disk structure surrounding the central bulge, but no distinct spiral arms or prominent star-forming regions are discernible in the image. The outer regions of the galaxy fade gradually into the background sky, with no obvious signs of tidal disturbances or recent merger events.
