The galaxy presents as a luminous, elliptical or spheroidal structure. It appears largely featureless, with a smooth, centrally concentrated light profile. There is a dominant, roundish core which fades gradually into the outer regions. The color is generally yellow with a possible increase in redder hues toward the galaxy’s core. There is no apparent spiral structure or evidence of a significant, blue star-forming disk. Based on the observed morphology, this galaxy is likely a relatively massive system dominated by an older stellar population, potentially located at a distance that causes faint disturbances to not be easily observed. There may be evidence of a tidal interaction or minor merger event, indicated by a subtle distortion or plume-like feature in the outer halo of the galaxy, but more detailed imaging would be required to confirm this.
