The galaxy presents a generally elliptical morphology, although some features suggest a disk component may also be present. A bright, concentrated central bulge is visible, characterized by a yellowish-white hue, suggestive of an older stellar population. Diffuse, fainter material surrounds the central bulge, extending outwards in a somewhat flattened distribution. There appears to be a slight bluing of the outer regions of the galaxy, indicating some ongoing, albeit likely low-level, star formation. Faint, non-distinct arm structures are very subtly suggested in the blue regions. There is no evidence of any major merger events or significant tidal disturbances in this image, though a subtle asymmetry suggests a minor interaction cannot be entirely ruled out. The galaxy has a red shift, thus it is relatively distant.
