The galaxy exhibits a generally elliptical morphology, with a bright, concentrated central bulge. There is an apparent disk component, though it is less pronounced and appears somewhat irregular. The galaxy presents an overall smooth appearance, although there is some evidence of faint, diffuse features which may represent spiral arms or tidal disturbances. The color distribution is fairly uniform, with a slight reddening towards the central bulge, suggesting an older stellar population in that region. There is a blueish tinge around the edges of the disk which could indicate a younger, hotter stellar population with ongoing or recent star formation. The disk appears to be at a slight angle relative to our line of sight. No strong dust lanes or prominent star-forming regions are immediately apparent. The galaxy appears fairly massive and is likely to be relatively evolved.
