The galaxy presents a relatively smooth, elliptical morphology. Its color profile suggests a dominance of older stellar populations, with a redder hue indicating less ongoing star formation activity. The object appears compact, with no apparent spiral arm structure or prominent dust lanes. A slight elongation is visible, suggesting a deviation from a perfectly spherical shape. There may be evidence of a faint extended halo surrounding the main body of the galaxy, but this is difficult to ascertain definitively from the image. No significant tidal disturbances or signs of recent merger activity are readily apparent. The galaxy displays a moderate level of intrinsic luminosity.
