The galaxy presents a largely smooth, elliptical morphology. There is a concentrated central bulge that dominates the galaxy's overall appearance, exhibiting a yellowish hue, indicative of an older stellar population. Faint, diffuse outer regions extend from the central bulge, gradually fading into the background. There is little to no visible dust lane or spiral arm structure. The shape is neither perfectly spherical nor highly elongated, appearing somewhere in between round and elliptical. There is no strong visual evidence of any recent or ongoing major merger events or significant tidal disturbances. Any minor disturbances are subtle, suggesting a relatively quiescent state. The light profile suggests a high degree of central concentration. Based on the color and smooth morphology, this galaxy is likely a relatively massive system with a suppressed star formation rate.
