The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated central bulge with a distinct yellowish hue, suggestive of an older stellar population. The galaxy fades gradually into the background with no distinct, sharp edges to the galactic disk. There appears to be minimal, if any, evidence of spiral arm structure or active star formation regions within the visible light spectrum. The overall morphology indicates a system approaching quiescence in terms of star formation activity. There may be some subtle disturbances that are causing a slight visual irregularity. The galaxy appears to be somewhat round and not cigar-shaped. It does not seem to be undergoing any major merger activity.
