The galaxy presents a largely smooth morphology, with a concentrated central bulge that appears approximately round in shape. The overall color profile suggests a dominant population of older stars, contributing to the observed yellowish hue. There is a subtle extension in the galaxy's light distribution, deviating slightly from a perfectly circular form, indicating the presence of either a weak disk-like component or some tidal disturbance, though evidence for significant mergers is not immediately apparent. Low levels of recent star formation are suspected. The galaxy exhibits a moderate redshift value suggesting that it resides at a significant cosmological distance. Based on its characteristics, this is likely a massive elliptical galaxy at an estimated distance of 4.4 kpc, with log solar mass of approximately 11.