The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggesting a population of older, evolved stars. There is a faint, extended halo surrounding the core, displaying a gradual decrease in luminosity with increasing radius. No distinct spiral arms or dust lanes are visible, which supports the conclusion that the galaxy is likely an elliptical galaxy with a relatively low ongoing star formation rate. The overall structure appears undisturbed, indicating a lack of recent major merger events. Its apparent color indices show a redder spectral energy distribution, consistent with a galaxy dominated by an older stellar population and a relatively low rate of star formation. The galaxy is approximately 6.5 kpc in radius.
