The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. There is a lack of any immediately discernible spiral arm structure or pronounced dust lanes. The light distribution appears even, with a gradual decrease in intensity from the core outwards. The color profile suggests an older stellar population with a redder hue, possibly indicating a diminished rate of ongoing star formation. There's no clear evidence of tidal features or strong gravitational interactions, suggesting it is relatively undisturbed. The overall appearance points towards a mature galaxy, possibly an elliptical or lenticular type.