The galaxy presents as a centrally concentrated object with a generally smooth light distribution. The core region exhibits a bright, slightly elongated structure, possibly indicative of an active galactic nucleus or a dense stellar population. There's a subtle color gradient visible, with a slightly redder hue towards the central region, potentially due to a higher concentration of older stars or dust obscuration. No distinct spiral arms or prominent star-forming regions are discernible from the image. Faint hints of an extended halo or tidal features could be present, but the image resolution limits further characterization. The overall morphology suggests a mature, early-type galaxy, possibly elliptical or lenticular, with little evidence of ongoing major star formation. There appears to be some sign of a possible merger with a companion galaxy, though it is difficult to say for sure with this data.
