The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. There are only some disturbances to the galaxy's form. There is a lack of distinct spiral arm structures or a prominent disk. The light distribution suggests that the galaxy is composed primarily of older stars, as evidenced by its yellow-reddish hue, potentially indicating lower levels of current star formation activity. The galaxy has a red shift of about 0.25, so it is fairly far from our own. There is evidence of a possible minor disturbance, such as some asymmetric structure, or tidal features, and the galaxy is likely not involved in a major merger event.
