The galaxy presents as a centrally concentrated object with a relatively smooth overall morphology.  It exhibits an elliptical appearance with an approximate axial ratio suggesting it is closer to round than highly elongated.  The central region displays a significantly higher surface brightness, appearing almost unresolved and exhibiting a yellowish hue. This color likely indicates a population of older stars dominating the nuclear region.  Fainter, bluer light is observed in the outer regions.  There are no obvious spiral arms or bar structures visible in this image, nor is there any evidence of a major ongoing merger or tidal disturbances. Faint extensions may be present, but are difficult to resolve with clarity.
