The galaxy exhibits a roughly elliptical morphology, although some degree of disk-like structure is suggested. The central region displays a bright, concentrated core. Extending outward from the core, there appears to be a fainter, more diffuse halo or envelope. There are faint, possible arm-like extensions, or tidal debris. The color distribution is complex. The core shows a yellow tint, possibly indicative of an older stellar population. The surrounding region transitions to a bluer hue, which might indicate the presence of younger stars or active star formation. There are possible signs of minor disturbance or irregularity in the structure, though no obvious signs of a major merger.
