The galaxy appears to be an elliptical type, exhibiting a generally smooth, spheroidal morphology. There is a noticeable central bulge that seems to be quite prominent and concentrated, displaying a yellowish hue, indicative of an older stellar population. Fainter light extends outwards from the core. The light distribution across the galaxy's body is generally smooth, with no obvious spiral arm structures or dust lanes visible. It is elongated, with the major axis being several times longer than the minor axis. There may be a very faint, diffuse outer envelope surrounding the main body of the galaxy. There are potential signs of tidal disturbance or interactions, showing the presence of a slightly asymmetrical light distribution. Overall, the galaxy's color is relatively uniform, suggesting a lack of significant ongoing star formation throughout the galaxy, with the central region being dominated by older, redder stars.
