The galaxy presents a relatively smooth, elliptical morphology. There is a centrally concentrated luminosity gradient, with a bright, unresolved core that diminishes gradually into its outer regions. The isophotes are close to elliptical. There is little evidence of a spiral arm structure, dust lanes, or other significant morphological features, suggesting that it is likely an early-type galaxy. The galaxy appears to be slightly elongated along a specific axis, displaying an inclination angle that indicates it is not perfectly face-on. The color profile suggests a higher concentration of older stellar populations. The overall appearance of the galaxy indicates it is likely a quiescent system with relatively low levels of ongoing star formation.
