The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated central bulge. The disk component is subtle, but perceptible, revealing a flattened shape. The disk is oriented at a notable inclination relative to our line of sight. The galaxy's color profile indicates a population of older stars, evidenced by a reddish hue in the central regions. The outer regions of the galaxy appear bluer, suggesting the presence of younger, hotter stars and ongoing, but faint, star formation. The overall luminosity indicates a galaxy of substantial mass. There is no clear evidence of any major recent mergers. The overall impression is of a well-formed galaxy, likely in a relatively quiescent state.
