The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. A slight elongation is perceptible, diverging marginally from a perfectly circular form. The galaxy exhibits a yellow-red hue, suggestive of an older stellar population with lower rates of recent star formation. It is relatively compact, but the central bulge has a high concentration of light. There appears to be a minor disturbance in the galaxy's morphology. This could potentially be due to a minor merger event or tidal interactions, which is causing a distortion in the galaxy's structure.
