The galaxy presents as a centrally concentrated, smooth distribution of light. There is a subtle ellipticity to its overall shape; it is neither perfectly spherical nor highly elongated. Its color appears to be consistent across the galaxy, with a slight reddish hue. This may indicate an older stellar population dominating the luminosity output. There are no obvious signs of spiral arms, dust lanes, or significant star-forming regions. The absence of significant irregularities or asymmetries suggests that this is likely a relaxed system, with no ongoing major mergers or interactions significantly distorting its morphology. The galaxy is not particularly compact and the light distribution fades gradually towards the outskirts. Overall, the appearance is that of a relatively massive, evolved system.
