The galaxy presents a generally smooth, elliptical morphology. Its central region appears as a concentrated, bright yellow-white bulge. Moving outwards, there is a subtle color gradient transitioning from yellow-white in the core to a slightly greenish hue in the outer regions. This may indicate the presence of some ongoing star formation, although it is not very prominent. No distinct spiral arms or bar structures are visible. The overall structure suggests an evolved system, potentially nearing the end of its star-forming activity. There is very slight distortion of the light on the edges of the galaxy, possibly indicating a minor interaction or disturbance. The overall roundness of the galaxy indicates that it may be close to an E4 or E5 type galaxy on the Hubble Sequence.
