The galaxy presents a generally smooth, rounded morphology. Its color profile suggests a higher concentration of older stellar populations, with a yellowish central bulge dominating the light output. There is some evidence of a faint, diffuse disk component extending outwards. A very slight asymmetry is observed, possibly indicating a minor interaction or internal disturbance, though the overall structure appears largely undisturbed. The limited bluer light hints at a low ongoing star formation rate. Estimated size suggests a large, massive system.
