The galaxy presents as a primarily smooth, elliptical structure with a concentrated, bright central bulge. The object exhibits an overall yellowish-orange hue, suggesting an older stellar population and a relative lack of ongoing star formation. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy is approximately circular in appearance, with only a slight elongation. No significant tidal disturbances or nearby merging companions are immediately apparent, suggesting a dynamically relaxed system.
