The galaxy appears to be an elliptical galaxy, showing a generally smooth and featureless morphology. It is characterized by a bright, concentrated central region, potentially indicative of a dense stellar population or an active galactic nucleus, surrounded by a less luminous, more diffuse halo. The overall shape is nearly elliptical but leans towards being in between round and cigar shaped. There are no visible spiral arms or distinct dust lanes, suggesting a lack of significant ongoing star formation. A slight color gradient is apparent, with the central region exhibiting a yellowish hue, possibly indicating older stellar populations and lower rates of star formation, transitioning to a redder hue as it moves outwards. There is no evidence of major mergers or significant tidal disturbances affecting the galaxy's structure although minor disturbances are possible.
