The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core, suggestive of a significant stellar population density. The luminosity decreases gradually towards the outer regions. The overall color profile appears to be slightly red, with a hint of yellow, suggestive of an older stellar population with less ongoing star formation. No distinct spiral arms or bar structures are discernible. There is no evidence of significant tidal disturbances or interactions with other galaxies. A slight elongation is observed, deviating marginally from a perfect circular shape.
