The galaxy presents as a moderately luminous, elliptical structure. The central region exhibits a concentrated and bright core, suggesting a higher density of stars in that area. The overall color profile appears relatively uniform across the galaxy, shifting slightly towards the redder end of the spectrum. This could be indicative of an older stellar population. The morphology is smooth, with no obvious spiral arm structures or significant dust lanes. It shows a generally undisturbed form, with no immediate signs of ongoing major merger activity. It has a moderate size and is well-defined, lacking significant tidal distortion or interaction features with other nearby galaxies.
