The object presents as a galaxy with a smooth, concentrated central bulge, exhibiting a yellowish hue, potentially indicating an older stellar population. The galaxy appears generally elliptical in shape, with a moderate degree of roundness. There is faint evidence of a surrounding disk component, suggested by the slight flattening of the galaxy's overall profile. The arms, if present, are not well defined. No significant tidal disturbances or signs of major merging events are readily apparent; though a possible minor disturbance cannot be ruled out based on the image. The lack of distinct blue regions suggests relatively low current star formation activity. The overall color suggests the galaxy is dominated by older stars.
