The galaxy presents a generally smooth and centralized morphology. The central region appears to be dominated by older stellar populations, exhibiting a yellowish hue, with a spheroidal shape. The outer regions show a gradual decrease in surface brightness. There is little evidence of distinct spiral arm structure or significant dust lanes. Faint blue regions are present along the outer edges of the galaxy, suggesting some ongoing low-level star formation. The galaxy does not show evidence of any major mergers or significant tidal disturbances and seems to be of intermediate size.
