The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a concentrated, bright luminosity, with a color profile indicating a likely older stellar population. Moving outward from the center, there's a gradual decrease in surface brightness. Hints of bluer hues are discernible in the outer regions, suggesting the presence of some younger stars. The overall morphology is elongated, appearing cigar-shaped, with no obvious signs of spiral arms or major disturbances from mergers. There's a slight asymmetry in the outer isophotes, which might indicate a minor interaction or past accretion event. No strong dust lanes or prominent star-forming regions are immediately apparent, which may indicate a relatively low rate of current star formation.
