The galaxy appears to be an elliptical galaxy, characterized by a smooth, nearly round morphology. There is no discernible spiral arm structure or significant dust lanes. The galaxy exhibits a bright, concentrated central bulge, with the luminosity gradually decreasing towards the outer edges. Its color suggests a moderate population of older stars, with a general lack of blue hues, indicating a comparatively lower rate of on-going star formation. There is no apparent tidal disturbance or ongoing merger activity visible, suggesting it is relatively isolated and undisturbed.
