The galaxy presents a largely smooth morphology, suggesting it is likely an elliptical galaxy, or possibly a spiral galaxy viewed face-on with a dominant bulge. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The galaxy appears somewhat elongated, deviating from a perfectly circular shape. There are no clearly discernible spiral arms or prominent dust lanes. The color is primarily yellowish, indicative of a stellar population dominated by older, redder stars, but with a significant enough blue component implying that active, though low, star formation is present. There are no signs of major mergers or significant tidal disturbances, but a slight irregularity could indicate a minor interaction.
