The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that emits a significant amount of light. There is little evidence of defined spiral arms or intricate dust lanes. The light appears to be of an orange/red hue, indicative of an older stellar population dominated by cooler, redder stars. There may be a very faint disk component, with a slight elongation to the galaxy shape, but any features are not well-defined. There are possible indications of minor disturbances, perhaps from a previous or ongoing interaction, however the general structure appears mostly undisturbed. 
