The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a dominant, rounded central bulge, characterized by a yellow-orange hue, suggesting an older stellar population. There's a slight elongation to the galaxy, possibly indicating a weak disk-like structure or a mild tidal interaction, though no distinct spiral arms are discernible. A faint blueish tint is visible around the perimeter of the bulge, possibly indicating more recent star formation activity. The galaxy shows no signs of major mergers or significant tidal disturbances.
