The galaxy appears as a relatively compact object, exhibiting a slightly elliptical morphology. The light distribution suggests a dominant, centrally concentrated bulge component, with a smoother appearance indicative of an older stellar population. There's faint evidence of a very weak disk, if one exists at all. The galaxy displays a yellowish-orange hue overall, suggesting a dearth of recent star formation and a population dominated by older, redder stars. There's an absence of any clearly defined spiral arm structures or prominent dust lanes. There are very faint hints of minor disturbances in the immediate vicinity of the galaxy.
