This galaxy presents as a relatively smooth, elliptical or lenticular system at a redshift of approximately 0.29. The light profile is dominated by a central bulge, exhibiting a concentrated luminosity in the core region. There appears to be little to no resolved spiral structure or prominent dust lanes. Color gradients suggest a redder, likely older stellar population dominating the galaxy's composition. The galaxy does not show signs of any major mergers or tidal disturbances; any interactions would likely be minor or ongoing. It is difficult to determine its exact shape and features without further observation but it is likely fairly round and undisturbed.
