The galaxy appears to be a relatively bright object with a smooth, elliptical morphology. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The core region exhibits a slightly brighter, more compact structure. There is a slight extension of luminosity along the horizontal axis, hinting at a mild deviation from perfect circularity. No distinct spiral arms or prominent dust lanes are discernible within the galaxy's structure. Faint hints of disturbances or irregularities are present, though the overall form is not drastically affected. There is an appearance of a merger in progress, though it may be a minor interaction. The galaxy is redder in the center than its surrounding regions, perhaps indicating the presence of older stars.