The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. It exhibits a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars. The light distribution appears spheroidal and relatively round, with no obvious disk structure or spiral arms visible. There is no evidence of significant ongoing star formation within the galaxy, although the presence of bluer light indicates a very low level of current star formation in a small region close to the center. There are no apparent tidal features or signs of recent mergers or interactions with other galaxies.
