The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth morphology with a high degree of central concentration. The light profile suggests a relatively homogenous stellar population. It displays a yellowish-orange hue, indicative of older stars and a lack of significant ongoing star formation. The galaxy appears somewhat rounded in shape, though there is a subtle elongation that may suggest a transition toward a more lenticular morphology. The galaxy's radial light distribution appears to be regular, showing no evidence of significant tidal features or interactions with neighboring galaxies. There are no clearly discernible spiral arms or a prominent disk component within the central region of the galaxy. The object exhibits an estimated physical size in the range of a few kiloparsecs, suggesting it is a galaxy of moderate size.
