The galaxy presents a largely smooth morphology, with an elliptical shape dominating the visual structure. The color profile suggests a concentration of older stellar populations, exhibiting a reddish hue in the central regions. There's little evidence of prominent spiral arms or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of major mergers or tidal disturbances, though a slight asymmetry might indicate minor interactions. Its overall appearance is consistent with an early-type galaxy, likely an elliptical, with a relatively low star formation rate. The elongated form suggests a possible transition between E and S0 type galaxies.
