The galaxy presents a somewhat elliptical morphology, appearing moderately smooth with a dominant central bulge region. Within this region, a concentration of light suggests an active galactic nucleus or a dense stellar population. There are subtle irregularities in the outer regions of the galaxy which may suggest minor gravitational disturbances or tidal interactions with nearby galaxies. The colour profile is predominantly yellow and red, indicating a relatively low rate of current star formation and a prevalence of older stellar populations. However, some blue regions also exist, suggesting ongoing star formation in some areas.
