The galaxy presents a largely smooth, elliptical morphology. Its overall shape is relatively round, with only a slight deviation towards a cigar shape. There is evidence of some disturbances, though no major merger is visibly occurring. The galaxy has a luminous core, suggesting the presence of an active galactic nucleus or a dense stellar population. The overall color appears to be leaning towards the redder end of the spectrum, hinting at a potentially older stellar population with lower star formation activity. There is an apparent smooth distribution of light throughout, indicative of a lack of spiral arm structure or distinct star-forming regions.
