The galaxy exhibits a somewhat elliptical morphology, appearing neither perfectly spherical nor distinctly disk-like. The light distribution is brightest and most concentrated towards the center, gradually fading outwards, suggesting a prominent bulge. There is a subtle asymmetry present in the light distribution, with a faint extension or plume visible towards the upper left quadrant. The overall color profile appears relatively uniform, trending towards a slightly redder hue. There is a faint blueish region to the upper left, indicating recent star formation. A lack of clearly defined spiral arms or a distinct disk structure suggests that the galaxy may be classified as an elliptical or lenticular type, although the subtle disturbances indicate that it may have undergone a minor merger.
