The galaxy appears as a centrally concentrated, elliptical system, exhibiting a smooth light distribution with no obvious spiral arms or disk-like features. The galaxy possesses an overall round morphology, lacking any significant elongation or cigar-like shape. There is no indication of ongoing major mergers or significant tidal disturbances. Its color suggests a population of older stars, with a higher concentration of redder wavelengths, implying a relatively low ongoing star formation rate. The galaxy has a luminous core surrounded by a less bright halo. There is a faint blueish haze, possibly indicating some star formation. 
