The galaxy presents a generally smooth morphology with a slight elongation. Its shape is primarily elliptical, appearing more "in-between" than distinctly round or cigar-shaped. There is no prominent central bulge, spiral arm structure, or bar. Some possible minor distortions are present. The galaxy has a red hue, suggesting a stellar population dominated by older, redder stars. There's little evidence of on-going, significant star formation activity. The light is relatively evenly distributed across the galaxy, indicative of a well-mixed stellar population. There is no indication of a major merger or significant tidal disruption. The galaxy is reasonably compact in size.
