The galaxy presents as a somewhat elliptical object, exhibiting a smooth overall morphology. There is a distinct central bulge region that appears brighter and more concentrated. The light distribution falls off gradually from the center, with no obvious spiral arm structures visible. There appears to be evidence of tidal disturbances or minor interactions, with a hint of asymmetry in the outer regions and a possible faint arm or plume extending from one side. The galaxy’s color suggests a stellar population with a mix of older stars, particularly in the bulge, as indicated by the redder hues, with younger, bluer stars possibly in the disrupted arm area. The light distribution indicates that this galaxy could potentially be undergoing a merging process.
