The galaxy presents as a generally smooth, rounded object. The light distribution appears centrally concentrated, exhibiting a bright core that fades gradually outwards. There is little evidence of distinct spiral arms or bar structures. The colour profile is suggestive of an older stellar population, the galaxy appears yellow/orangeish. While it mainly appears as a single, unperturbed object, there is a nearby object that may indicate a minor disturbance, such as a very small merging event, although it is difficult to say with certainty. It does not appear particularly active in terms of star formation based on the available data.
