The galaxy presents as an elongated, somewhat cigar-shaped object. It is characterized by a centrally concentrated bulge region exhibiting a reddish hue, possibly indicative of an older stellar population. The overall structure appears relatively smooth with a high degree of symmetry, although there might be very subtle indications of minor structural disturbances. A faint blueish tinge is visible at the outer edges of the galaxy, which is consistent with some regions of ongoing, although limited, star formation. There is no strong indication of a prominent disk or spiral arm structure. The galaxy does not appear to be undergoing any major merging events or significant tidal interactions.
