The galaxy presents as a single, largely featureless, and centrally concentrated object. It has a generally round morphology. The dominant coloration is a yellow-orange hue, suggesting a stellar population composed of older, less massive stars. There appears to be a fainter blue tinge to the periphery of the object, perhaps indicating a faint area of more recent star formation activity. No distinct spiral arms or bar structures are discernible in the image. There is a neighboring blue object to the left of the main galaxy, and its relation is unclear. It could be a small irregular galaxy in the background, or a tidal dwarf galaxy in the process of formation. There is no obvious evidence of a major ongoing merger, although minor disturbances may be present. The general lack of distinct features suggests the galaxy is likely an elliptical or lenticular type, dominated by an older stellar population.
