The galaxy presents a generally smooth morphology. The central region exhibits a bright, concentrated core, indicative of a substantial stellar population and possibly an active galactic nucleus. The overall shape appears largely rounded, with a slight deviation from perfect circularity, suggesting a possible ellipsoidal structure. A faint, diffuse disk is present surrounding the central bulge, extending outwards. There is some evidence of faint, spiral arm-like features within the disk but these are poorly defined. There are some indications of minor tidal disturbances to the north of the galaxy, suggesting a past interaction or merger event. The galaxy exhibits a range of colors, with a bluer hue in the outer regions, possibly indicating ongoing star formation, and a redder hue towards the center, suggesting an older stellar population.
