The galaxy presents a generally smooth morphology with a notable absence of distinct spiral arms or a prominent bar structure. Its shape is somewhat elliptical, appearing more elongated than perfectly circular. The central region exhibits a brighter, concentrated luminosity, suggesting a significant stellar density, likely a bulge component. The galaxy's color profile indicates a predominantly older stellar population, with a yellowish-red hue. There is no strong evidence of ongoing major star formation regions within the visible spectrum. A subtle asymmetry, perhaps a slight distortion in the outer regions, may suggest a past or ongoing minor interaction with another galaxy, however the overall structure appears to be relatively settled.
