The galaxy exhibits an elliptical morphology, appearing smooth with a centrally concentrated light distribution. The color profile suggests an aging stellar population, with a redder hue in the central bulge transitioning to slightly bluer tones at the outer edges. The galaxy displays a notable tilt relative to our line of sight, implying a somewhat flattened spheroidal shape. No distinct spiral arms or active star-forming regions are readily apparent. Minor disturbances may be present within the galaxy due to a possible recent merging event or tidal interaction.
