The galaxy presents as a slightly elongated, lenticular or elliptical structure. It exhibits a relatively smooth light distribution, lacking prominent spiral arms or distinct dust lanes. There is some subtle suggestion of a central bulge. The galaxy's color profile is primarily redder in hue, indicating a population of older stars, with a small population of young stars. There's no strong indication of ongoing, vigorous star formation within the visible region, consistent with a relatively quiescent state. The observed morphology suggests the galaxy may be in a later stage of its evolutionary timeline, having potentially undergone past mergers or interactions that have disrupted its structure. However, there are no obvious signs of recent major merger events. Faintly lit and a good distance away, this galaxy is a faint smudge in the cosmos.
