The galaxy presents as a luminous, relatively compact object. Its overall morphology appears somewhat elliptical, exhibiting a centrally concentrated brightness profile indicative of a significant bulge component. The color is generally yellowish, suggesting a stellar population dominated by older, redder stars and a low rate of on-going star formation. There may be a slight asymmetry or disturbance in its outer regions, possibly hinting at past or ongoing interactions. Some evidence of diffuse features is seen, but no clearly defined spiral arms are apparent.
