This galaxy exhibits a generally smooth morphology, appearing largely spheroidal in shape with high central concentration. The light distribution suggests a single, dominant component with no obvious spiral arms or bar structure visible. The galaxy presents a rounded appearance, with a slight elongation. There is little to no evidence of ongoing major merging activity, though minor disturbances cannot be ruled out due to the image quality. Based on its color profile, the galaxy's stellar population is likely dominated by older, redder stars, potentially indicating a relatively low current star formation rate. The object demonstrates a relatively uniform structure suggesting a classification as an elliptical galaxy.
