The galaxy presents as a relatively compact object, exhibiting a somewhat smooth morphology. There is a noticeable concentration of light towards the central region, with a gradual decrease in intensity towards the outer edges. The overall shape approximates a flattened spheroid, leaning towards an elliptical form rather than a distinct spiral. The light appears largely homogenous across the galaxy, lacking prominent features such as defined spiral arms or significant dust lanes. There may be subtle irregularities within the galaxy's outer regions, suggesting possible minor gravitational disturbances. The color profile seems to show a slightly redder hue, possibly implying an older stellar population and suppressed star formation activity.
