The galaxy presents as a moderately inclined disk, with a noticeably brighter central bulge. The overall color profile indicates a population dominated by older stars, evidenced by the yellowish-white hue observed across the galaxy. However, there is evidence of ongoing, albeit relatively low, star formation, particularly discernible through the presence of bluer regions in the disk component. The disk exhibits some irregularities, possibly indicative of minor gravitational disturbances. The galaxy’s shape is neither perfectly elliptical nor distinctly spiral, suggesting a morphology somewhere between an elliptical and a spiral galaxy. One notable feature is a small, reddish extension emanating from one side of the disk, potentially a tidal tail or an area of concentrated H-alpha emission. The galaxy is relatively compact, with no obvious signs of a major ongoing merger or significant disruption.
