The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The galaxy exhibits a generally round shape. There is a slight elongation but it is largely contained in the central region. The color profile indicates the presence of older stellar populations, showing a yellow-red hue. Faint hints of bluer regions at the edges may indicate some ongoing, but relatively low, star formation. There are no significant tidal features, strong dust lanes, or other indications of recent major merger activity. There may be evidence of minor disturbances but further inspection is needed. The galaxy appears to be relatively isolated in this field.
