The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light distribution suggests a single component with no discernible spiral arms or bar structure. The core region presents a brighter, more intense luminosity, gradually decreasing in intensity towards the outer edges. The overall color profile indicates a relatively red population, implying an older stellar population with limited ongoing star formation. There is no significant evidence of tidal disturbances or merging activity in the immediate vicinity of the galaxy. The galaxy's appearance is largely undisturbed, suggesting it is a relatively isolated system.
