The galaxy presents a smooth, elliptical morphology. It appears largely featureless with no apparent spiral arms or prominent dust lanes visible at this resolution. The light distribution is concentrated towards the center, exhibiting a bright, well-defined core that suggests a significant central mass concentration. The overall color is yellowish-orange, which implies a stellar population dominated by older, redder stars and a relatively low rate of ongoing star formation. The shape is nearly circular. There is no evidence of any major ongoing merger activity or significant tidal disturbances affecting the galaxy's structure.
