The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a somewhat elongated, cigar-like shape. There is a bright, concentrated central bulge. The galaxy's light profile appears to fade gradually from the center outwards, with no distinct spiral arm features visible. The color profile suggests a galaxy dominated by older stellar populations, with a redder hue overall. There is no evidence of any major ongoing merging activity or significant disturbances in its structure, although some minor asymmetries cannot be ruled out. The galaxy appears to be relatively isolated, without any other nearby galaxies in the immediate vicinity to suggest tidal interactions.
