The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. The light distribution appears relatively uniform, lacking prominent spiral arm structures or a distinct bar. The core of the galaxy exhibits a brighter, more condensed luminosity profile, potentially indicative of an active galactic nucleus or a dense stellar population. The overall color is skewed toward the redder end of the spectrum. This, combined with the galaxy's smooth appearance, implies an older stellar population with suppressed star formation activity. There may be slight distortions visible around the edges that could indicate minor interactions with smaller satellite galaxies or a tidal disturbance.
