The galaxy presents a moderately smooth morphology. The central region exhibits a concentrated, bright yellowish hue, suggesting an older stellar population. The overall shape appears somewhat elliptical, though it is closer to being in between round and cigar shaped, without a strong disk component. Hints of bluer, less concentrated regions are seen in the outer areas, potentially indicating younger star formation. There may be some minor disturbances in the galaxy's structure that are not clearly visible. Overall, the galaxy appears to be a relatively massive system at a considerable distance, with moderate star formation activity.
